Strong-coupling theory of magnetic-exciton-mediated superconductivity in UPd$_2$Al$_3$

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磁共振(磁谐振耦合)无线充电技术鼻祖级文章-英文原文

磁共振(磁谐振耦合)无线充电技术鼻祖级文章-英文原文

Wireless Power Transfer via Strongly Coupled Magnetic ResonancesAndré Kurs,1* Aristeidis Karalis,2 Robert Moffatt,1 J. D. Joannopoulos,1 Peter Fisher,3Marin Soljačić11Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. 2Department of Electrical Engineering and Computer Science, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. 3Department of Physics and Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.*To whom correspondence should be addressed. E-mail: akurs@Using self-resonant coils in a strongly coupled regime, we experimentally demonstrate efficient non-radiative power transfer over distances of up to eight times the radius of the coils. We demonstrate the ability to transfer 60W with approximately 40% efficiency over distances in excess of two meters. We present a quantitative model describing the power transfer which matches the experimental results to within 5%. We discuss practical applicability and suggest directions for further studies. At first glance, such power transfer is reminiscent of the usual magnetic induction (10); however, note that the usual non- resonant induction is very inefficient for mid-range applications.Overview of the formalism. Efficient mid-range power transfer occurs in particular regions of the parameter space describing resonant objects strongly coupled to one another. Using coupled-mode theory to describe this physical system (11), we obtain the following set of linear equationsIn the early 20th century, before the electrical-wire grid, Nikola Tesla (1) devoted much effort towards schemes to a&m(t)=(iωm-Γm)a m(t)+∑iκmn a n(t)+F m(t)n≠m(1)transport power wirelessly. However, typical embodiments (e.g. Tesla coils) involved undesirably large electric fields. During the past decade, society has witnessed a dramatic surge of use of autonomous electronic devices (laptops, cell- phones, robots, PDAs, etc.) As a consequence, interest in wireless power has re-emerged (2–4). Radiative transfer (5), while perfectly suitable for transferring information, poses a number of difficulties for power transfer applications: the efficiency of power transfer is very low if the radiation is omnidirectional, and requires an uninterrupted line of sight and sophisticated tracking mechanisms if radiation is unidirectional. A recent theoretical paper (6) presented a detailed analysis of the feasibility of using resonant objects coupled through the tails of their non-radiative fields for mid- range energy transfer (7). Intuitively, two resonant objects of the same resonant frequency tend to exchange energy efficiently, while interacting weakly with extraneous off- resonant objects. In systems of coupled resonances (e.g. acoustic, electro-magnetic, magnetic, nuclear, etc.), there is often a general “strongly coupled” regime of operation (8). If one can operate in that regime in a given system, the energy transfer is expected to be very efficient. Mid-range power transfer implemented this way can be nearly omnidirectional and efficient, irrespective of the geometry of the surrounding space, and with low interference and losses into environmental objects (6).Considerations above apply irrespective of the physical nature of the resonances. In the current work, we focus on one particular physical embodiment: magnetic resonances (9). Magnetic resonances are particularly suitable for everyday applications because most of the common materials do not interact with magnetic fields, so interactions with environmental objects are suppressed even further. We were able to identify the strongly coupled regime in the system of two coupled magnetic resonances, by exploring non-radiative (near-field) magnetic resonant induction at MHzfrequencies. where the indices denote the different resonant objects. The variables a m(t) are defined so that the energy contained in object m is |a m(t)|2, ωm is the resonant frequency of thatisolated object, and Γm is its intrinsic decay rate (e.g. due to absorption and radiated losses), so that in this framework anuncoupled and undriven oscillator with parameters ω0 and Γ0 would evolve in time as exp(iω0t –Γ0t). The κmn= κnm are coupling coefficients between the resonant objects indicated by the subscripts, and F m(t) are driving terms.We limit the treatment to the case of two objects, denoted by source and device, such that the source (identified by the subscript S) is driven externally at a constant frequency, and the two objects have a coupling coefficient κ. Work is extracted from the device (subscript D) by means of a load (subscript W) which acts as a circuit resistance connected to the device, and has the effect of contributing an additional term ΓW to the unloaded device object's decay rate ΓD. The overall decay rate at the device is therefore Γ'D= ΓD+ ΓW. The work extracted is determined by the power dissipated in the load, i.e. 2ΓW|a D(t)|2. Maximizing the efficiency η of the transfer with respect to the loading ΓW, given Eq. 1, is equivalent to solving an impedance matching problem. One finds that the scheme works best when the source and the device are resonant, in which case the efficiency isThe efficiency is maximized when ΓW/ΓD= (1 + κ2/ΓSΓD)1/2. It is easy to show that the key to efficient energy transfer is to have κ2/ΓSΓD> 1. This is commonly referred to as the strongcoupling regime. Resonance plays an essential role in thisDS S D'' power transfer mechanism, as the efficiency is improved by approximately ω2/ΓD 2 (~106 for typical parameters) compared to the case of inductively coupled non-resonant objects. Theoretical model for self-resonant coils. Ourexperimental realization of the scheme consists of two self- resonant coils, one of which (the source coil) is coupled inductively to an oscillating circuit, while the other (the device coil) is coupled inductively to a resistive load (12) (Fig. 1). Self-resonant coils rely on the interplay between distributed inductance and distributed capacitance to achieve resonance. The coils are made of an electrically conducting wire of total length l and cross-sectional radius a wound into Given this relation and the equation of continuity, one finds that the resonant frequency is f 0 = 1/2π[(LC )1/2]. We can now treat this coil as a standard oscillator in coupled-mode theory by defining a (t ) = [(L /2)1/2]I 0(t ).We can estimate the power dissipated by noting that the sinusoidal profile of the current distribution implies that the spatial average of the peak current-squared is |I 0|2/2. For a coil with n turns and made of a material with conductivity σ, we modify the standard formulas for ohmic (R o ) and radiation (R r ) µ0ω l a helix of n turns, radius r , and height h . To the best of our knowledge, there is no exact solution for a finite helix in the literature, and even in the case of infinitely long coils, the solutions rely on assumptions that are inadequate for our R o = 2σ 4πa µ πωr 42 ωh 2 (6)system (13). We have found, however, that the simple quasi- R =0 n 2 + (7)static model described below is in good agreementr ε 12 c3π3 c(approximately 5%) with experiment.We start by observing that the current has to be zero at the ends of the coil, and make the educated guess that the resonant modes of the coil are well approximated bysinusoidal current profiles along the length of the conducting wire. We are interested in the lowest mode, so if we denote by s the parameterization coordinate along the length of the conductor, such that it runs from -l /2 to +l /2, then the time- dependent current profile has the form I 0 cos(πs /l ) exp(i ωt ). It follows from the continuity equation for charge that the linear charge density profile is of the form λ0 sin(πs /l ) exp(i ωt ), so the two halves of the coil (when sliced perpendicularly to its axis) contain charges equal in magnitude q 0 = λ0l /π but opposite in sign.As the coil is resonant, the current and charge density profiles are π/2 out of phase from each other, meaning that the real part of one is maximum when the real part of the other is zero. Equivalently, the energy contained in the coil is 0The first term in Eq. 7 is a magnetic dipole radiation term(assuming r << 2πc /ω); the second term is due to the electric dipole of the coil, and is smaller than the first term for our experimental parameters. The coupled-mode theory decay constant for the coil is therefore Γ = (R o + R r )/2L , and its quality factor is Q = ω/2Γ.We find the coupling coefficient κDS by looking at the power transferred from the source to the device coil,assuming a steady-state solution in which currents and charge densities vary in time as exp(i ωt ).P =⎰d rE (r )⋅J (r ) =-⎰d r (A&S (r )+∇φS (r ))⋅J D (r ) at certain points in time completely due to the current, and at other points, completely due to the charge. Usingelectromagnetic theory, we can define an effective inductance L and an effective capacitance C for each coil as follows:=-1⎰⎰d r d r ' µJ &S(r ')+ρS(r ') 4π |r -r |ε0≡-i ωMI S I Dr '-r|r '-r |3⋅J D (r )(8)L =µ04π |I 0 |⎰⎰d r d r 'J (r )⋅J (r ')|r -r '|where the subscript S indicates that the electric field is due to the source. We then conclude from standard coupled-mode theory arguments that κDS = κSD = κ = ωM /2[(L S L D )1/2]. When 1 1 ρ(r )ρ(r ') the distance D between the centers of the coils is much larger= C 4πε 0 |q 0 | ⎰⎰d r d r ' |r -r '|(4)than their characteristic size, κ scales with the D -3dependence characteristic of dipole-dipole coupling. Both κ and Γ are functions of the frequency, and κ/Γ and the where the spatial current J (r ) and charge density ρ(r ) are obtained respectively from the current and charge densities along the isolated coil, in conjunction with the geometry of the object. As defined, L and C have the property that the efficiency are maximized for a particular value of f , which is in the range 1-50MHz for typical parameters of interest. Thus, picking an appropriate frequency for a given coil size, as we do in this experimental demonstration, plays a major role in optimizing the power transfer.1 2Comparison with experimentallydeterminedU =2 L |I 0 |parameters. The parameters for the two identical helical coils built for the experimental validation of the power 1 2 transfer scheme are h = 20cm, a = 3mm, r = 30 cm, and n = =2C|q 0 | (5)5.25. Both coils are made of copper. The spacing between loops of the helix is not uniform, and we encapsulate theuncertainty about their uniformity by attributing a 10% (2cm) uncertainty to h . The expected resonant frequency given these22dimensions is f0 = 10.56 ± 0.3MHz, which is about 5% off from the measured resonance at 9.90MHz.The theoretical Q for the loops is estimated to be approximately 2500 (assuming σ = 5.9 × 107 m/Ω) but the measured value is Q = 950±50. We believe the discrepancy is mostly due to the effect of the layer of poorly conductingcopper oxide on the surface of the copper wire, to which the current is confined by the short skin depth (~20μm) at this frequency. We therefore use the experimentally observed Q and ΓS= ΓD= Γ = ω/2Q derived from it in all subsequent computations.We find the coupling coefficient κ experimentally by placing the two self-resonant coils (fine-tuned, by slightly adjusting h, to the same resonant frequency when isolated) a distance D apart and measuring the splitting in the frequencies of the two resonant modes. According to coupled-mode theory, this splitting should be ∆ω = 2[(κ2-Γ2)1/2]. In the present work, we focus on the case where the two coils are aligned coaxially (Fig. 2), although similar results are obtained for other orientations (figs. S1 and S2).Measurement of the efficiency. The maximum theoretical efficiency depends only on the parameter κ/[(L S L D)1/2] = κ/Γ, which is greater than 1 even for D = 2.4m (eight times the radius of the coils) (Fig. 3), thus we operate in the strongly- coupled regime throughout the entire range of distances probed.As our driving circuit, we use a standard Colpitts oscillator whose inductive element consists of a single loop of copper wire 25cm in radius(Fig. 1); this loop of wire couples inductively to the source coil and drives the entire wireless power transfer apparatus. The load consists of a calibrated light-bulb (14), and is attached to its own loop of insulated wire, which is placed in proximity of the device coil and inductively coupled to it. By varying the distance between the light-bulb and the device coil, we are able to adjust the parameter ΓW/Γ so that it matches its optimal value, given theoretically by (1 + κ2/Γ2)1/2. (The loop connected to the light-bulb adds a small reactive component to ΓW which is compensated for by slightly retuning the coil.) We measure the work extracted by adjusting the power going into the Colpitts oscillator until the light-bulb at the load glows at its full nominal brightness.We determine the efficiency of the transfer taking place between the source coil and the load by measuring the current at the mid-point of each of the self-resonant coils with a current-probe (which does not lower the Q of the coils noticeably.) This gives a measurement of the current parameters I S and I D used in our theoretical model. We then compute the power dissipated in each coil from P S,D=ΓL|I S,D|2, and obtain the efficiency from η = P W/(P S+ P D+P W). To ensure that the experimental setup is well described by a two-object coupled-mode theory model, we position the device coil such that its direct coupling to the copper loop attached to the Colpitts oscillator is zero. The experimental results are shown in Fig. 4, along with the theoretical prediction for maximum efficiency, given by Eq. 2. We are able to transfer significant amounts of power using this setup, fully lighting up a 60W light-bulb from distances more than 2m away (figs. S3 and S4).As a cross-check, we also measure the total power going from the wall power outlet into the driving circuit. The efficiency of the wireless transfer itself is hard to estimate in this way, however, as the efficiency of the Colpitts oscillator itself is not precisely known, although it is expected to be far from 100% (15). Still, the ratio of power extracted to power entering the driving circuit gives a lower bound on the efficiency. When transferring 60W to the load over a distance of 2m, for example, the power flowing into the driving circuit is 400W. This yields an overall wall-to-load efficiency of 15%, which is reasonable given the expected efficiency of roughly 40% for the wireless power transfer at that distance and the low efficiency of the Colpitts oscillator.Concluding remarks. It is essential that the coils be on resonance for the power transfer to be practical (6). We find experimentally that the power transmitted to the load drops sharply as either one of the coils is detuned from resonance. For a fractional detuning ∆f/f0 of a few times the inverse loaded Q, the induced current in the device coil is indistinguishable from noise.A detailed and quantitative analysis of the effect of external objects on our scheme is beyond the scope of the current work, but we would like to note here that the power transfer is not visibly affected as humans and various everyday objects, such as metals, wood, and electronic devices large and small, are placed between the two coils, even in cases where they completely obstruct the line of sight between source and device (figs. S3 to S5). External objects have a noticeable effect only when they are within a few centimeters from either one of the coils. While some materials (such as aluminum foil, styrofoam and humans) mostly just shift the resonant frequency, which can in principle be easily corrected with a feedback circuit, others (cardboard, wood, and PVC) lower Q when placed closer than a few centimeters from the coil, thereby lowering the efficiency of the transfer.When transferring 60W across 2m, we calculate that at the point halfway between the coils the RMS magnitude of the electric field is E rms= 210V/m, that of the magnetic field isH rms= 1A/m, and that of the Poynting vector is S rms=3.2mW/cm2 (16). These values increase closer to the coils, where the fields at source and device are comparable. For example, at distances 20cm away from the surface of the device coil, we calculate the maximum values for the fields to be E rms= 1.4kV/m, H rms= 8A/m, and S rms= 0.2W/cm2. The power radiated for these parameters is approximately 5W, which is roughly an order of magnitude higher than cell phones. In the particular geometry studied in this article, the overwhelming contribution (by one to two orders of magnitude) to the electric near-field, and hence to the near- field Poynting vector, comes from the electric dipole moment of the coils. If instead one uses capacitively-loaded single- turn loop design (6) - which has the advantage of confining nearly all of the electric field inside the capacitor - and tailors the system to operate at lower frequencies, our calculations show (17) that it should be possible to reduce the values cited above for the electric field, the Poynting vector, and the power radiated to below general safety regulations (e.g. the IEEE safety standards for general public exposure(18).) Although the two coils are currently of identical dimensions, it is possible to make the device coil small enough to fit into portable devices without decreasing the efficiency. One could, for instance, maintain the product of the characteristic sizes of the source and device coils constant, as argued in (6).We believe that the efficiency of the scheme and the power transfer distances could be appreciably improved by silver-plating the coils, which should increase their Q, or by working with more elaborate geometries for the resonant objects (19). Nevertheless, the performance characteristics of the system presented here are already at levels where they could be useful in practical applications.References and Notes1. N. Tesla, U.S. patent 1,119,732 (1914).2.J. M. Fernandez, J. A. Borras, U.S. patent 6,184,651(2001).3.A. Esser, H.-C. Skudelny, IEEE Trans. Indust. Appl. 27,872(1991).4.J. Hirai, T.-W. Kim, A. Kawamura, IEEE Trans. PowerElectron. 15, 21(2000).5.T. A. Vanderelli, J. G. Shearer, J. R. Shearer, U.S. patent7,027,311(2006).6.A. Karalis, J. D. Joannopoul os, M. Soljačić, Ann. Phys.,10.1016/j.aop.2007.04.017(2007).7.Here, by mid-range, we mean that the sizes of the deviceswhich participate in the power transfer are at least a few times smaller than the distance between the devices. For example, if the device being powered is a laptop (size ~ 50cm), while the power source (size ~ 50cm) is in thesame room as the laptop, the distance of power transfer could be within a room or a factory pavilion (size of the order of a fewmeters).8. T. Aoki, et al., Nature 443, 671 (2006).9.K. O’Brien, G. Scheible, H. Gueldner, 29th AnnualConference of the IEEE 1, 367(2003).10.L. Ka-Lai, J. W. Hay, P. G. W., U.S. patent7,042,196(2006).11.H. Haus, Waves and Fields in Optoelectronics(Prentice- Supporting Online Material/cgi/content/full/1143254/DC1SOM TextFigs. S1 to S530 March 2007; accepted 21 May 2007Published online 7 June 2007; 10.1126/science.1143254 Include this information when citing this paper.Fig. 1. Schematic of the experimental setup. A is a single copper loop of radius 25cm that is part of the driving circuit, which outputs a sine wave with frequency 9.9MHz. S and D are respectively the source and device coils referred to in the text. B is a loop of wire attached to the load (“light-bulb”). The various κ’s represent direct couplings between the objects indicated by the arrows. The angle between coil D and the loop A is adjusted to ensure that their direct coupling is zero, while coils S and D are aligned coaxially. The direct couplings between B and A and between B and S are negligible.Fig. 2. Comparison of experimental and theoretical values for κ as a function of the separation between coaxially aligned source and device coils (the wireless power transfer distance.) Fig. 3. Comparison of experimental and theoretical values for the parameter κ/Γ as a function of the wireless power transfer distance. The theory values are obtained by using the theoretical κ and the experimentally measured Γ. The shaded area represents the spread in the theoretical κ/Γ due to the 5% uncertainty in Q.Fig. 4. Comparison of experimental and theoretical efficiencies as functions of the wireless power transfer distance. The shaded area represents the theoretical prediction for maximum efficiency, and is obtained by inserting theHall, Englewood Cliffs, NJ, 1984).12.The couplings to the driving circuit and the load donot theoretical values from Fig. 3 into Eq. 2 [with Γκ2/Γ2 1/2 W /ΓD= (1 +have to be inductive. They may also be connected by awire, for example. We have chosen inductive coupling in the present work because of its easier implementation. 13.S. Sensiper, thesis, Massachusetts Institute of Technology(1951).14.We experimented with various power ratings from 5W to75W.15.W. A. Edson, Vacuum-Tube Oscillators (Wiley, NewYork,1953).16.Note that E ≠cμ0H, and that the fields are out of phaseand not necessarily perpendicular because we are not in a radiativeregime.17.See supporting material on Science Online.18.IEEE Std C95.1—2005 IEEE Standard for Safety Levelswith Respect to Human Exposure to Radio FrequencyElectromagnetic Fields, 3 kHz to 300 GHz (IEEE,Piscataway, NJ,2006).19. J. B. Pendry, Science 306, 1353 (2004).20. The authors would like to thank John Pendry forsuggesting the use of magnetic resonances, and Michael Grossman and Ivan Čelanović for technical assistance.This work was supported in part by the Materials Research Science and Engineering Center program of the National Science Foundation under Grant No. DMR 02-13282, by the U.S. Department of Energy under Grant No. DE-FG02-99ER45778, and by the Army Research Officethrough the Institute for Soldier Nanotechnologies under Contract No. DAAD-19-02-D0002.) ]. The black dots are the maximum efficiency obtained from Eq. 2 and the experimental values of κ/Γ from Fig. 3. The red dots present the directly measured efficiency,as described in thetext.。

磁学 径向克尔 英文 kerr effect

磁学 径向克尔 英文 kerr effect

IntroductionThe Kerr effect, also known as the magneto-optic Kerr effect (MOKE), is a phenomenon that manifests the interaction between light and magnetic fields in a material. It is named after its discoverer, John Kerr, who observed this effect in 1877. The radial Kerr effect, specifically, refers to the variation in polarization state of light upon reflection from a magnetized surface, where the change occurs radially with respect to the magnetization direction. This unique aspect of the Kerr effect has significant implications in various scientific disciplines, including condensed matter physics, materials science, and optoelectronics. This paper presents a comprehensive, multifaceted analysis of the radial Kerr effect, delving into its underlying principles, experimental techniques, applications, and ongoing research directions.I. Theoretical Foundations of the Radial Kerr EffectA. Basic PrinciplesThe radial Kerr effect arises due to the anisotropic nature of the refractive index of a ferromagnetic or ferrimagnetic material when subjected to an external magnetic field. When linearly polarized light impinges on such a magnetized surface, the reflected beam experiences a change in its polarization state, which is characterized by a rotation of the plane of polarization and/or a change in ellipticity. This alteration is radially dependent on the orientation of the magnetization vector relative to the incident light's plane of incidence. The radial Kerr effect is fundamentally governed by the Faraday-Kerr law, which describes the relationship between the change in polarization angle (ΔθK) and the applied magnetic field (H):ΔθK = nHKVwhere n is the sample's refractive index, H is the magnetic field strength, K is the Kerr constant, and V is the Verdet constant, which depends on the wavelength of the incident light and the magnetic properties of the material.B. Microscopic MechanismsAt the microscopic level, the radial Kerr effect can be attributed to twoprimary mechanisms: the spin-orbit interaction and the exchange interaction. The spin-orbit interaction arises from the coupling between the electron's spin and its orbital motion in the presence of an electric field gradient, leading to a magnetic-field-dependent modification of the electron density distribution and, consequently, the refractive index. The exchange interaction, on the other hand, influences the Kerr effect through its role in determining the magnetic structure and the alignment of magnetic moments within the material.C. Material DependenceThe magnitude and sign of the radial Kerr effect are highly dependent on the magnetic and optical properties of the material under investigation. Ferromagnetic and ferrimagnetic materials generally exhibit larger Kerr rotations due to their strong net magnetization. Additionally, the effect is sensitive to factors such as crystal structure, chemical composition, and doping levels, making it a valuable tool for studying the magnetic and electronic structure of complex materials.II. Experimental Techniques for Measuring the Radial Kerr EffectA. MOKE SetupA typical MOKE setup consists of a light source, polarizers, a magnetized sample, and a detector. In the case of radial Kerr measurements, the sample is usually magnetized along a radial direction, and the incident light is either p-polarized (electric field parallel to the plane of incidence) or s-polarized (electric field perpendicular to the plane of incidence). By monitoring the change in the polarization state of the reflected light as a function of the applied magnetic field, the radial Kerr effect can be quantified.B. Advanced MOKE TechniquesSeveral advanced MOKE techniques have been developed to enhance the sensitivity and specificity of radial Kerr effect measurements. These include polar MOKE, longitudinal MOKE, and polarizing neutron reflectometry, each tailored to probe different aspects of the magnetic structure and dynamics. Moreover, time-resolved MOKE setups enable the study of ultrafast magneticphenomena, such as spin dynamics and all-optical switching, by employing pulsed laser sources and high-speed detection systems.III. Applications of the Radial Kerr EffectA. Magnetic Domain Imaging and CharacterizationThe radial Kerr effect plays a crucial role in visualizing and analyzing magnetic domains in ferromagnetic and ferrimagnetic materials. By raster-scanning a focused laser beam over the sample surface while monitoring the Kerr signal, high-resolution maps of domain patterns, domain wall structures, and magnetic domain evolution can be obtained. This information is vital for understanding the fundamental mechanisms governing magnetic behavior and optimizing the performance of magnetic devices.B. Magnetometry and SensingDue to its sensitivity to both the magnitude and direction of the magnetic field, the radial Kerr effect finds applications in magnetometry and sensing technologies. MOKE-based sensors offer high spatial resolution, non-destructive testing capabilities, and compatibility with various sample geometries, making them suitable for applications ranging from magnetic storage media characterization to biomedical imaging.C. Spintronics and MagnonicsThe radial Kerr effect is instrumental in investigating spintronic and magnonic phenomena, where the manipulation and control of spin degrees of freedom in solids are exploited for novel device concepts. For instance, it can be used to study spin-wave propagation, spin-transfer torque effects, and all-optical magnetic switching, which are key elements in the development of spintronic memory, logic devices, and magnonic circuits.IV. Current Research Directions and Future PerspectivesA. Advanced Materials and NanostructuresOngoing research in the field focuses on exploring the radial Kerr effect in novel magnetic materials, such as multiferroics, topological magnets, and magnetic thin films and nanostructures. These studies aim to uncover newmagnetooptical phenomena, understand the interplay between magnetic, electric, and structural order parameters, and develop materials with tailored Kerr responses for next-generation optoelectronic and spintronic applications.B. Ultrafast Magnetism and Spin DynamicsThe advent of femtosecond laser technology has enabled researchers to investigate the radial Kerr effect on ultrafast timescales, revealing fascinating insights into the fundamental processes governing magnetic relaxation, spin precession, and all-optical manipulation of magnetic order. Future work in this area promises to deepen our understanding of ultrafast magnetism and pave the way for the development of ultrafast magnetic switches and memories.C. Quantum Information ProcessingRecent studies have demonstrated the potential of the radial Kerr effect in quantum information processing applications. For example, the manipulation of single spins in solid-state systems using the radial Kerr effect could lead to the realization of scalable, robust quantum bits (qubits) and quantum communication protocols. Further exploration in this direction may open up new avenues for quantum computing and cryptography.ConclusionThe radial Kerr effect, a manifestation of the intricate interplay between light and magnetism, offers a powerful and versatile platform for probing the magnetic properties and dynamics of materials. Its profound impact on various scientific disciplines, coupled with ongoing advancements in experimental techniques and materials engineering, underscores the continued importance of this phenomenon in shaping our understanding of magnetism and driving technological innovations in optoelectronics, spintronics, and quantum information processing. As research in these fields progresses, the radial Kerr effect will undoubtedly continue to serve as a cornerstone for unraveling the mysteries of magnetic materials and harnessing their potential for transformative technologies.。

强磁防蜡节能器技术探索与应用

强磁防蜡节能器技术探索与应用

1目前现状清蜡是保证机采井正常生产的主要措施,按照清蜡方式不同,分为三类:一是热清蜡,利用热传导,达到融蜡的目的;二是物理清蜡,即机械清蜡[1-3],是指专门的工具刮除油管壁和抽油杆上的蜡,并靠液流将蜡带至地面的清蜡方法;三是辅助清蜡,以物理或化学性质的工具、药剂等,阻止蜡的形成与结晶[4],从而达到防蜡的目的。

通过调查,因热洗能力不足、热洗管线距离过长、热洗管线频繁穿孔问题,造成某厂1324口井热洗效果不佳、热洗无法按计划周期执行[5]。

所以强磁防蜡节能器技术探索与应用于济源公杰(大庆油田有限责任公司第六采油厂)摘要:某油田进入高含水开发后期,采出原油具有“双高”(含蜡高、含水率高)特性。

在机采管理上,由于洗井不及时、套喷生产、关井时间长等原因,导致部分井的管、杆结蜡,严重时油管、套管均会出现蜡卡堵现象。

应用强磁防蜡器可有效减少因结蜡导致的油井产量下降、能耗升高、泵况异常等问题,现场试验结果表明强磁防蜡器能够有效降低蜡质的形成及附着,起到了良好的降黏及抑制蜡晶的作用,最高可降低原油黏度40%左右,降低结蜡率30%,达到了清蜡、防蜡的目的,预计全年可节电50×104kWh,节省用电成本40万元,实现了节能防蜡的效果。

关键词:清蜡;强磁防蜡;原油黏度;节能;治理DOI :10.3969/j.issn.2095-1493.2023.08.006Exploration and application of energy conservation technology for strong magnetic wax prevention YU Jiyuan,GONG JieNO.6Oil Production Plant of Daqing Oilfield Co .,Ltd .Abstract:An oilfield has entered the late stage of high water content development,and the crude oil produced has the characteristics of "double high"(high wax content and high water content).In terms of mechanical production management,due to untimely well flushing,casing blowout production,long shut-in time and other reasons,some well pipes and rods are waxed,and both tubing and casing will be stuck with wax in serious cases.The strong magnetic wax prevention technology should be ap-plied to effectively reduce the decline in well production,increase in energy consumption and pump inspection problems caused by wax.The field experiment results show that the strong magnetic wax preventer can be effectively reduced the formation and adhesion of wax,and has a good effect of re-ducing viscosity and inhibiting the formation of wax crystals.The maximum viscosity of crude oil can be reduced by 40%,and the wax deposition rate can be reduced by 30%,which achieves the purpose of wax removal and wax prevention.It is estimated that the power saving of the whole year can be saved 50×104kWh,saved electricity costs of 400000yuan,and achieved the effect of energy conser-vation and wax prevention .Keywords:wax removal;strong magnetic wax prevention;crude oil viscosity;energy conserva-tion;treatment第一作者简介:于济源,工程师,2013年毕业于八一农垦大学(机械设计制造及其自动化专业),从事采油工程举升设备管理及井下作业材料管理工作,132****0671,****************,黑龙江省大庆油田第六采油厂工艺研究所,163114。

毕业设计(论文)-X射线C型臂系统结构设计(全套图纸三维)

毕业设计(论文)-X射线C型臂系统结构设计(全套图纸三维)

毕业设计(论文)-X射线C型臂系统结构设计(全套图纸三维)毕业设计说明书题目名称:X射线C型臂系统结构设计说明书院系名称:机械设计制造及其自动化班级:学号:学生姓名:指导教师:2015年3月摘要本课题来源于当今社会医疗工业医疗康复设备的创新和更新换代基础之上,通过设计出X射线C型臂系统结构,从而来满足当今社会医疗、康复设备不足的缺陷。

国内X射线C型臂系统结构的研发及制造要与全球号召的高效经济、治疗效果好,效率高等主题保持一致。

近期对医疗机械行业中X射线C型臂系统结构的使用情况进行了调查,发现在医疗机械行业中,X射线C型臂的使用非常普遍。

自然而然在医疗机械设备中它们的安装也非常频繁。

传统的X射线C型臂使用难度大,对病人身体的检测的程度不够,价格昂贵,所以设计一个新型的X射线C型臂系统结构势在必行。

本文运用大学所学的知识,提出了X射线C型臂系统结构组成、工作原理以及主要零部件的设计中所必须的理论计算和相关强度校验,构建了X射线C型臂系统结构总的指导思想,从而得出了该X射线C型臂系统结构的优点是高效,经济,并且使用方便等结论。

关键字:医疗机械、X射线C型臂系统,设备,高效全套图纸,加153893706AbstractWith development of all kind of science technology and global economy, Pneumatic manipulator is a automated devices that can mimic the human hand and arm movements to do something,aslo can according to a fixed procedure to moving objects or control tools.Therefore widely used in machine building, metallurgy, electronics, light industry and atomic energy sectors.The pneumatic part of the design is primarily to choose the right valves and design a reasonable pneumatic control loop, by controlling and regulating pressure, flow atcompressedneceengththdirectionprocedurework.The inverted pendulum is a typical high order system, with multi variable, non-linea r, strong-coupling, fleet and absolutely instable. It is representative as an ideal model to prove new control theory and techniques. During the control process, pendulum can effec tively reflect many key problems such as equanimity, robust, follow-up and track, therefo re.This paper studies a control method of double inverted pendulum . First of all, the mat hematical model of the double inverted pendulum is established, then make a control desi gn to double inverted pendulum on the mathematical model, and determine the system pe rformance index weightmatrix , by using genetic algorithm in order to attain the system s tate feedback control matrix. Finally, the simulation of the system is made by .Key word: pneumatic manipulator cylinder pneumatic loop Fout degrees of freedom.目录摘要 (I)Abstract (II)1 引言 (1)1.1 课题的来源与研究的目的和意义 (1)1.2 C臂X射线机的用途 (2)1.3 C臂X射线机的特点 (1)1.4 本课题研究的内容 (3)1.5 Solidworks设计基础 (4)1.5.1 草图绘制 (5)1.5.2 基准特征,参考几何体的创建 (6)1.5.3 拉伸、旋转、扫描和放样特征建 (7)1.5.4 工程图的设计 (10)1.5.5 装配设计 (11)2 X射线C型臂系统结构总体结构的设计 (12)2.1 X射线C型臂系统结构的总体方案图 (12)2.2 X射线C型臂系统结构的工作原理 (15)2.3 X射线C型臂系统结构的设计计算 (17)2.3.1CCD摄像机的选型计算 (18)2.3.2转动轴的设计计算 (19)2.3.3轴承的选型计算 (19)3 各主要零部件强度的校核 (21)3.1转动轴强度的校核与计算 (22)3.2轴承强度的校核计算 (23)4 X射线C型臂系统结构中主要零件的三维建模 (24)4.1控制柜的三维建模 (25)4.2底架的三维建模 (25)4.3脚轮的三维建模 (27)4.4 C臂X射线机的三维建模 (28)5 三维软件设计总结 (29)结论 (30)致谢 (31)参考文献 (32)1 引言1.1课题的来源与研究的目的和意义机械工业是国民的装备部,是为国民经济提供装备和为人民生活提供耐用消费品的产业。

基于matlab的永磁同步电机调速系统的仿真

基于matlab的永磁同步电机调速系统的仿真

摘要本文首先介绍了永磁同步电机的国内外发展状况,然后介绍了永磁同步电机的结构及原理,接着建立了永磁同步电机的数学模型,并在此基础上用MATLAB 进行了仿真,最后进行了仿真及仿真结果的分析。

永磁同步电机是具有非线性、强耦合性、时变性的系统,在运行过程中会受到负载扰动等多因素影响。

以往研究永磁同步电机的做法是在硬件上搭建一个平台进行模拟,但是这样在做实验中难免会造成一些损失,而且硬件上的反馈会比较长研究周期长。

目前在国内外关于永磁同步电机调速系统的研究现状上来讲,基于MATLAB环境下仿真模型的构建下进行研究,这可极大的缩短研究周期和研究成本。

在利用MATLAB仿真模型研究永磁同步电机时,我们可以把那些扰动因数做成模拟信号给予模型,这样可以准确的定性分析实验得出结论。

关键字:永磁同步电机,空间矢量调制,MATLAB仿真,数学模型。

ABSTRACTIn the first, this paper introduces the domestic and international development status of Permanent Magnet Synchronous Motor(PMSM), gives a explanation about its basictheory, structure. Then it builds a mathematical model, and uses MATLAB to simulate that model.The PMSM is a nonlinear, strong-coupling and time-varying system, so in the operation process, it will be influenced by many factors such asload disturbance. Therere, it is necessary to take action when researching the control method of PMSM. The former research method is setting up a platform on hardware to perform experimensbut it is undesirable, because it often cause some loss, and the feedback cycle is longer than research cycle. As fordomestic and international current situation on the research of PMSM, it is obvious that researching under the simulation model created by MATLAB could greatly reduce the cost and cycle of researchment. When using MATLAB to build simulation model on the research of PMSM, we can transform these disturbance factors into analog signal, making a qualitative analysis to draw conclusions from them.Keywords:PMSM, SVPWM, MATLAB simulation, mathmatical model目录摘要 (I)ABSTRACT .............................................. I I 目录............................................... I II 第一章绪论 (1)1.1 研究背景及意义 (1)1.1.1 研究背景 (1)1.1.2 研究的目的及意义 (1)1.2 国内外研究现状 (2)1.2.1 国内研究历史及现状 (2)1.2.2 国外研究现状及趋势 (2)1.3 本文的主要内容 (3)第二章永磁同步电机调速系统的结构和数学模型 (5)2.1 引言 (5)2.2 永磁同步电机调速系统的结构 (5)2.3 永磁同步电机调速系统的数学模型 (6)2.3.1 PMSM在ABC坐标系下的磁链和电压方程 (6)坐标系下的磁链和电压方程 (8)2.3.2 PMSM在02.3.3 PMSM在dq0坐标系下的磁链和电压方程 (9)2.4 永磁同步电机的控制策略 (11)2.5 本章小节 (12)第三章永磁同步电机矢量控制及空间矢量脉宽调制 (14)3.1 引言 (14)3.2 永磁同步电动机的矢量控制 (14)3.3 空间矢量脉宽调制概念 (15)3.4 SVPWM模块的建立 (17)3.5 本章小结 (23)第四章基于Matlab的永磁同步调速系统仿真模型的建立 (24)4.1 引言 (24)4.2 MATLAB软件的介绍 (24)4.3永磁同步电机调速系统整体模型的建立 (25)4.4仿真参数调试及结果分析 (28)4.5本章小结 (29)第五章总结与展望 (30)5.1全文总结 (30)参考文献 (31)致谢 (33)第一章绪论1.1 研究背景及意义1.1.1 研究背景随着电力电子技术、微电子技术和现代电机控制理论的发展,交流调速系统逐步具备了宽调速范围、高稳速精度、快速动态响应及四象限运行等良好的技术性能,交流调速系统应用越来越广泛。

无线电传输在双线圈及四线圈系统中的耦合模理论

无线电传输在双线圈及四线圈系统中的耦合模理论

Transmission of Wireless Power in Two-Coil and Four-Coil Systems using Coupled Mode TheoryManasi Bhutada, Vikaram Singh, ChiragWartyDept. of Electrical and Electronics EngineeringIntelligent Communication LabMumbai, India无线电传输在双线圈及四线圈系统中的耦合模理论电气与电子工程系智能通信实验室印度,孟买姓名:学号:班级:日期:2016年7月2日Abstract—Wireless Power Transfer (WPT) systems are considered as sophisticated alternatives for modern day wired power transmission. Resonance based wireless power delivery is an efficient technique to transfer power over a relatively long distance. This paper presents a summary of a two-coil wireless power transfer system with the design theory, detailed formulations and simulation results using the coupled mode theory (CMT). Further by using the same theory, it explains the four-coil wireless power transfer system and its comparison with the two-coil wireless transfer power system. A four-coil energy transfer system can be optimized to provide maximum efficiency at a given operating distance. Design steps to obtain an efficient power transfer system are presented and a design example is provided. Further, the concept of relay is described and how relay effect can allow more distant and flexible energy transmission is shown.摘要——无线电源传输(WPT)系统被认为是复杂的现代有线输电的替代品。

PhysRevB.81.153104

PhysRevB.81.153104

Optical evidence of strong coupling between valence-band holes and d-localized spinsin Zn1−x Mn x OV.I.Sokolov,1A.V.Druzhinin,1N.B.Gruzdev,1A.Dejneka,2O.Churpita,2Z.Hubicka,2L.Jastrabik,2and V.Trepakov2,3 1Institute of Metal Physics,UD RAS,S.Kovalevskaya Str.18,620041Yekaterinburg,Russia2Institute of Physics,AS CR,v.v.i.,Na Slovance2,18221Praha8,Czech Republic3Ioffe Institute,RAS,194021St-Petersburg,Russia͑Received3December2009;revised manuscript received2March2010;published30April2010͒We report on optical-absorption study of Zn1−x Mn x O͑x=0–0.06͒films on fused silica substrates takingspecial attention to the spectral range of the fundamental absorption edge͑3.1–4eV͒.Well-pronounced exci-tonic lines observed in the region3.40–3.45eV were found to shift to higher energies with increasing Mnconcentration.The optical band-gap energy increases with x too,reliably evidencing strong coupling betweenoxygen holes and localized spins of manganese ions.In the3.1–3.3eV region the optical-absorption curve inthe manganese-containedfilms was found to shift to lower energies with respect to that for undoped ZnO.Theadditional absorption observed in this range is interpreted as a result of splitting of a localized Zhang-Rice-typestate into the band gap.DOI:10.1103/PhysRevB.81.153104PACS number͑s͒:78.20.ϪeI.INTRODUCTIONDilute magnetic semiconductor Zn1−x Mn x O is one of themost promising materials for the development of optoelec-tronic and spin electronic devices with ferromagnetism re-tained at practical temperatures͑i.e.,Ͼ300K͒.However,researchers are confronted with many complex problems.Ferromagnetic ordering does not always appear and the na-ture of its instability is a subject of controversy.In addition,optical properties of Zn1−x Mn x O appreciably differ fromthose in Zn1−x Mn x Se and Zn1−x Mn x S related compounds,where the intracenter optical transitions of Mn2+ions areconventionally observed in the optical-absorption and photo-luminescence spectra.1,2In contrast,a very intense absorp-tion in the2.2–3.0eV region was reported in Zn1−x Mn x Owithout any manifestations of intracenter transitions,3–5and photoluminescence due to4T1→6A1optical transition of Mn2+is absent as well.Interpretation of this absorption bandas a charge transfer3,5is complicated by the fact that Mn2+forms neither d5/d4donor nor d5/d6acceptor levels in the forbidden gap of ZnO.6,7To resolve this contradiction,Dietl8put forward the con-cept that the oxides and nitrides belong to the little studiedfamily of dilute magnetic semiconductors with strong corre-lations.Characteristic features of such compounds are an in-crease in the band gap with the concentration of magneticions and emergence of a Zhang-Rice͑Z-R͒-type state in theforbidden gap9arising as a result of strong exchange cou-pling of3d-localized spin of the impurity centers andvalence-band holes.According to Ref.8,fulfillment ofstrong hybridization condition depends on the ratio of theimpurity-center potential U to a critical value U c;a coupledhybrid state can be formed when U/U cϾ1.Existence of such electronic state has been verified by ab initio theoretical treatment of electron correlations using the local spin-density approximation͑LSDA+U model͒and calculation of the ex-change coupling values.10In Zn1−x Mn x O the hole can origi-nate by electron transfer from the Mn2+adjacent oxygen to the conduction band.The resulting hole localizes as the Z-R state leading to appearance of additional broad,intense ab-sorption band.In this way the study of optical-absorptionspectra can be used as a probe to identify the Z-R states.It is known that the optical band-edge absorption spec-trum of Mn-doped ZnO is characterized by the onset of astrong rise of the absorption coefficient in theϳ3.1eV spec-tral region.11In Refs.11and12,this absorption inZn1−x Mn x Ofilms was treated as a product of direct interbandoptical transitions using conventional formula␣2ϳ͑ប␻−E g͒.The resulting magnitudes of band gap for composition with x=0.05have been estimated as E g=3.10eV͑Ref.11͒and3.25eV,12which is appreciably less than E g=3.37eV inZnO.13Such“redshift”of the band gap was considered inRef.12as a result of p-d exchange interaction,in analogy tothe shift of the excitonic lines in reflectivity and lumines-cence spectra observed in Ref.14for Zn1−x Mn x Se.At thesame time theory predicts an increase in E g͑x͒with x for Zn1−x Mn x O.8Also excitonic absorption spectrum in Zn1−x Mn x O nanopowders,15appeared to be located at ener-gies higher than that in ZnO nanopowders,that does not confirm the shift of E g to lower energies for Zn1−x Mn x O films.In this work we report on the optical-absorption spectrastudies in thin Zn1−x Mn x Ofilms deposited on fused silicaing suchfilms we succeed to detect the absorp-tion spectra of excitons and to determine reliably the widthof the optical gap E g.This allowed us to elucidate the natureof the additional absorption band appearing atប␻ϽE g near the fundamental absorption edge as a result of splitting of one more Z-R-type state due to strong hybridization and ex-change coupling of3d-localized spin of the manganese and valence-band oxygen hole.II.EXPERIMENTALThin Zn1−x Mn x Ofilms with x=0–0.06,120–130,and 200–250nm of thicknesses were deposited on fused silica substrates by the atmospheric barrier-torch discharge tech-nique,as it was described in Refs.16and17.The substratePHYSICAL REVIEW B81,153104͑2010͒temperature during deposition was kept at ϳ200°C.Mn content was controlled by measurements of Mn and Zn emis-sion ͑␭em =4031Åand 4810Å,respectively ͒of plasma during deposition and crosschecked by the postgown EPMA ͑JEOL JXA-733device with Kevex Delta Class V mi-croanalyser ͒analysis with accuracy Ϯ0.3%.X-ray diffrac-tion ͑XRD ͒studies were performed with a Panalytical X’PertMRD Pro diffractometer with Eulerian cradle using Cu K ␣radiation ͑␭em =1.5405Å͒in the parallel beam ge-ometry.XRD profiles were fitted with the Pearson VII func-tion by the DIFPATAN code.18Correction for instrumental broadening was performed using NIST LaB6standard and V oigt function method.19Optical absorption within the 1.2–6.5eV spectral region was measured in unpolarized light at room temperature using a Shimadzu UV-2401PC spectrophotometer.The bare silica substrate and Zn 1−x Mn x O film on silica substrate were mounted into the reference and test channel,respectively.The optical density ␣d ͑product of optical-absorption coeffi-cient and film thickness ͒was calculated without taking into account multiple reflections as ␣d =ln ͑I 0/I ͒,where I 0and I are intensities of light passed through bare substrate and film/substrate structure.III.RESULTS AND DISCUSSIONFigure 1presents XRD pattern for ZnO and Zn 0.95Mn 0.05O films,as an example.All obtained films re-vealed crystalline block structure with dominant ͑002͒orien-tation of blocks’optical C -axes aligned normal to substrate.Observed reflexes correspond to wurtzite structure evi-dencing absence of extraneous phases.Both pure and Mn-doped ZnO films appeared to be compressively strained with 0.2%of strain,s =͑a 0−a S ͒/a 0,where a 0and a S are the lattice parameters of nonstrained and strained films.The analysis reveals that the value of compressive strain is controlled pre-dominantly by stresses,but not by presence of Mn ͑at least for Mn concentrations used ͒.Figure 2presents the optical-absorption spectra for Zn 1−x Mn x O films.A wide absorption line is seen in the re-gion of the band edge ͑Fig.2͒,whose energy appears to be shifted by about 100meV to higher energies in comparison with the excitonic line in ZnO ͓ϳ3.31eV at T =300K ͑Ref.13͔͒.The line shift is very likely connected with the com-pressive strain of Zn 1−x Mn x O films mentioned above.The wide and shifted line has been observed earlier in ZnO film on sapphire substrate 20,21and was identified as a shift of the excitonic line due to compressive strain of Zn 1−x Mn x O films.21The inset represents spectra of this line obtained in ZnO at T =300K and 77.3K.It is seen that the excitonic line is narrowed,split into two components and shifted to higher energies on lowering the temperature,clearly evidenc-ing its excitonic nature.The first line is a sum of A and B excitons,the second one is the C exciton appearing due to disorientation of blocks forming the film.16Analogous tem-perature evolutions have been reported for a wide excitonic line in ZnO nanocrystals.15As the concentration of Mn impurity increases,the exci-tonic line additionally broadens and shifts to higher energies.Figure 3shows the actual Mn concentration shift of the ex-citonic line energy ប␻exc .It is seen that the increase in Mn concentration leads to not only changes in the excitonic spec-trum but also exhibits enhancement of the band-gap energy in Zn 1−x Mn x O films ͑band-gap magnitude can be estimated as E g =ប␻exc +E exc ,where E exc =60meV is the excitonic binding energy 13͒.It is known that the band-gap magnitude in ZnO-MnO system varies from 3.37eV in ZnO up to 3.8eV in MnO.22According to the theoretical analysis 8per-formed taking into account inversion of ⌫7and ⌫9valence subbands in ZnO,23,24strong coupling of manganese spin and p states of valence band leads to appearance of a positiveI n t e n s i t y (c o u n t )2θ(degree)FIG.1.XRD pattern of ZnO ͑left scale ͒and Zn 0.95Mn 0.05O ͑right scale ͒films.E n e r g y (eV)αdFIG.2.Exciton absorption spectra of compressed Zn 1−x Mn x O films:1—x =0%,2—x =1.8%,and 3—x =5%;film thickness:d =͑120–130͒nm;and T =300K.Inset shows excitonic absorption lines for compressed ZnO:1—T =300K and 4—T =77.3K.01234563.403.413.423.433.44E n e r g y (e V )X (%)FIG.3.Mn-concentration dependence of the excitonic line en-ergies for Zn 1−x Mn x O films.additive in optical absorption of Zn 1−x Mn x O at small x val-ues.The sum of two contributions at sufficiently small x results in an increase in E g magnitude.The rise of the band-gap magnitude with the admixture of the second component E g ͑x ͒has been observed in Zn 1−x Co x O ͑Ref.25͒for exci-tonic lines registered in the reflection spectra at 1.6K.The shift of the excitonic line to higher energies was observed in Zn 0.99Fe 0.01O,too.20In the case of weak d -p coupling the additive into the band gap change appeared to be negative.8In this case the band-gap value E g decreases with x for x Յ0.1,as it was found for Zn 1−x Mn x Se ͑Fig.6in Ref.14͒and for Cd 1−x Mn x S.26Therefore,the observed rise of the E g ͑x ͒value with Mn addition provides the reliable experimental proof that the strong hybridization condition U /U c Ͼ1in Zn 1−x Mn x O is fulfilled.Figure 4presents optical absorption in Zn 1−x Mn x O films recorded in the spectral region 3.1–3.3eV .It is seen that the onset of optical absorption in Zn 1−x Mn x O films emerges at lower energies than that for ZnO ones.Analogous shift had been observed earlier in the spectrum of the photoluminescence excitation over deep im-purity centers in Zn 1−x Mn x O for Ref.15.Unlike authors of Refs.11and 12,we assume that addi-tional absorption of Zn 1−x Mn x O ͑in comparison with ZnO ͒in the 3.1–3.3eV range is a result of pushing the Z-R-type states out of valence band to the forbidden gap.9The essence of this state consists of localization of the valence-band hole within the first coordination sphere on the oxygen ions as a result of strong exchange interaction of manganese and hole spins.Such electronic state is similar to the Z-R-type state originally considered for La 2CuO 4oxidesuperconductor.9This state is a singlet one,because in La 2CuO 4the spins of d 9configuration of Cu 2+ion and oxy-gen holes are equal but of opposite direction.The situation is more complex in the case of Zn 1−x Mn x O since the top of valence band is formed by three close subbands:⌫7,⌫9,and ⌫7.23,24In such case we have serious reasons to assume that not only the presence of one deep Z-R-type state is respon-sible for optical absorption in the 2.2–3.0eV spectral region.We assume the presence of another,relatively shallow Z-R-type state too,which has been split off into the gap providing additional absorption in the 3.1–3.3eV region of Zn 1−x Mn x O.Tentatively,using results 11,12,15we estimate the splitting of the second Z-R level from the valence band as 0.12–0.27eV .More reliable determination of the split energy can be performed using more sensitive methods of absorp-tion spectra, e.g.,modulation methods,which are in progress.IV .CONCLUSIONThin Zn 1−x Mn x O films ͑x =0–0.06͒have been sintered and their optical-absorption spectra were investigated.The well-pronounced excitonic absorption lines in the fundamen-tal absorption spectral regions were observed.Position of excitonic absorption lines in Zn 1−x Mn x O films shifts to higher energies with increasing Mn content.This evidences an increase in the E g magnitude with x for small values x and reliably corroborates fulfillment of the strong coupling crite-rion ͑U /U c Ͼ1͒in Zn 1−x Mn x O.The last effect leads to emer-gence of an intense optical-absorption band in the 2.2–3.0eV region due to the presence of the band-gap Z-R-type state.The additional absorption observed in the range of 3.1–3.3eV is interpreted as a result of splitting of one more Z-R-type states into the band gap.ACKNOWLEDGMENTSAuthors thank T.Dietl,V .I.Anisimov,and A.V .Lukoy-anov for useful discussions and V .Valvoda for kind assis-tance in XRD experiments.This work was supported by Czech Grants No.A V0Z10100522of A V CR,No.KJB100100703of GA A V ,No.202/09/J017of GA CR,No.KAN301370701of A V CR,and No.1M06002of MSMT CR and Russian Grants No.08-02-99080r-ofiof RFBR,PP RAS “Quantum Physics of Condensed Matter”,and State Contract No.5162.nger and H.J.Richter,Phys.Rev.146,554͑1966͒.2T.Hoshina and H.Kawai,Jpn.J.Appl.Phys.19,267͑1980͒.3F.W.Kleinlein and R.Helbig,Z.Phys.266,201͑1974͒.4R.Beaulac,P.I.Archer,and D.R.Gamelin,J.Solid State Chem.181,1582͑2008͒.5T.Fukumura,Z.Jin,A.Ohtomo,H.Koinuma,and M.Kawasaki,Appl.Phys.Lett.75,3366͑1999͒.6K.A.Kikoin and V .N.Fleurov,Transition Metal Impurities in Semiconductors:Electronic Structure and Physical Properties ͑World Scientific,Singapore,1994͒,p.349.7T.Dietl,J.Magn.Magn.Mater.272-276,1969͑2004͒.8T.Dietl,Phys.Rev.B 77,085208͑2008͒.9F.C.Zhang and T.M.Rice,Phys.Rev.B 37,3759͑1988͒.10T.Chanier,F.Virot,and R.Hayn,Phys.Rev.B 79,205204͑2009͒.11V .Shinde,T.Gujar,C.Lokhande,R.Mane,and S.-H.Han,3.1253.2500.00.40.8αdEnergy (eV)12FIG.4.Spectral dependence of the optical density ␣d in the 3.1–3.3eV spectral region for Zn 1−x Mn x O,1—ZnO;2—x =0.3–0.5%;film thickness 200–250nm;and T =300K.Mater.Chem.Phys.96,326͑2006͒.12Y.Guo,X.Cao,n,C.Zhao,X.Hue,and Y.Song,J.Phys. Chem.C112,8832͑2008͒.13Zh.L.Wang,J.Phys.:Condens.Matter16,R829͑2004͒.14R.B.Bylsma,W.M.Becker,J.Kossut,U.Debska,and D. Yoder-Short,Phys.Rev.B33,8207͑1986͒.15V.I.Sokolov,A.Ye.Yermakov,M.A.Uimin,A.A.Mysik,V.A.Pustovarov,M.V.Chukichev,and N.B.Gruzdev,J.Lumin.129,1771͑2009͒.16M.Chichina,Z.Hubichka,O.Churpita,and M.Tichy,Plasma Processes Polym.2,501͑2005͒.17Z.Hubicka,M.Cada,M.Sicha,A.Churpita,P.Pokorny,L. Soukup,and L.Jastrabík,Plasma Sources Sci.Technol.11,195͑2002͒.18http://www.xray.cz/priv/kuzel/dofplatan/19R.Kuzel,Jr.,R.Cerny,V.Valvoda,and M.Blomberg,ThinSolid Films247,64͑1994͒.20Z.Jin,T.Fukumura,M.Kaasaki,K.Ando,H.Saito,T.Skiguchi, Y.Z.Yoo,M.Murakami,Y.Matsumoto,T.Hasegawa,and H. Koinuma,Appl.Phys.Lett.78,3824͑2001͒.21J.-M.Chauveau,J.Vives,J.Zuniga-Perez,ügt,M.Teis-seire,C.Deparis,C.Morhain,and B.Vinter,Appl.Phys.Lett.93,231911͑2008͒.d and V.E.Henrich,Phys.Rev.B38,10860͑1988͒. 23K.Shindo,A.Morita,and H.Kamimura,J.Phys.Soc.Jpn.20, 2054͑1965͒.24W.Y.Liang and A.D.Yoffe,Phys.Rev.Lett.20,59͑1968͒. 25W.Pacuski,D.Ferrand,J.Gibert,C.Deparis,J.A.Gaj,P.Ko-ssacki,and C.Morhain,Phys.Rev.B73,035214͑2006͒.26M.Ikeda,K.Itoh,and H.Sato,J.Phys.Soc.Jpn.25,455͑1968͒.。

光子阻塞效应

光子阻塞效应

学号:201105774题目名称: 强耦合下的光子阻塞效应研究题目类型: 研究论文学生姓名: 董昌瑞院(系): 物理与光电工程学院专业班级: 物理11102班指导教师: 邹金花辅导教师: 邹金花时间: 2015年1月至2015年6月目录毕业论文任务书` (I)指导教师评审意见 (VIII)评阅教师评语 (IX)答辩记录及成绩评定 (X)中文摘要 (XI)外文摘要 (XII)1引言 (1)2 基础理论知识 (1)2.1 光力振子系统 (1)2.2二能级原子与光场相互作用的全量子理论 (2)2.3光场关联函数 (5)2.4 光子计数统计 (8)3 模型方程与结果分析 (10)3.1模型方程 (10)3.2 方程分析 (12)4总结与展望 (14)参考文献 (14)致谢 (16)毕业论文任务书`院(系)物理与光电工程学院专业物理班级物理11102 学生姓名董昌瑞指导教师/职称邹金花/副教授1.毕业论文(设计)题目:强耦合下的光子阻塞效应研究2.毕业论文(设计)起止时间: 2015 年1月1 日~2015 年 6月10 日3.毕业论文(设计)所需资料及原始数据(指导教师选定部分)[1] A Ridolfo, M Leib, S Savasta, M J Hartmann. Photon Blockade in the Ultrastrong CouplingRegime [J]. Phys. Rev. Lett., 2012, 109: 193602-1~193602-5[2] Jieqiao Liao, C K Law. Cooling of a mirror in cavity optomechanics with a chirped pulse [J]. Phys. Rev. A, 2011, 84: 053838-1~053838-6[3] P Komar, S D Bennett, K Stannigel, S J M Habraken, P Rabl, P Zoller, M D Lukin. Single-photon nonlinearities in two-mode optomechanics [J]. Phys. Rev. A, 2013, 87: 013839-1~013839-10[4] T Ramos, V Sudhir, K Stannigel, P Zoller, T Kippenbrg. Nonlinear quantum optomechanics viaindividual intrinsic two-level defects [J]. Phys. Rev. Lett., 2013, 110: 193602-1~193602-5 [5] G Anetsberger, O Arcizet, Q P Unterreithmeier, R Riviere, A Schliesser, E M Weig, J P Kotthaus,T Kippenberg. Near-field cavity optomechanics with nanomechanical oscillators [J]. Nat. Phys., 2009, 5: 909~914[6] S J M Habraken, W Lechner, P Zoller. Resonances in dissipative optomechanics withnanoparticles: Sorting, speed rectification, and transverse coolings [J]. Phys. Rev. A, 2013, 87: 053808-1~053808-8[7] K Qu, G S Agarwal. Fano resonances and their control in optomechanics [J]. Phys. Rev. A, 2013,87: 063813-1~063813-7[8] A Nunnenkamp, K Borkje, S M Girvin. Cooling in the single-photon strong-coupling regime ofcavity optomechanics [J]. Phys. Rev. A, 2012, 85: 051803-1~051803-4[9] Y C Liu, Y F Xiao, X S Luan, C W Wong. Dynamic Dissipative Cooling of a MechanicalResonator in Strong Coupling Optomechanics [J]. Phys. Rev. A, 2013, 110: 153606-1~153606-5[10] A Nunnekamp, K Borkie, S M Girvin. Single-photon optomechanics [J]. Phys. Rev. Lett., 2011,107: 063602-1~063602-5[11] J M Dobrindt, I Wilson-Rae, T J Kippenbeg. Parametric Normal-Mode Splitting in CavityOptomechanics [J]. Phys. Rev. Lett., 2008, 101: 263602-1~263602-4[12]樊菲菲. 光力振子与原子间量子纠缠和振子压缩的研究[D]. 华中师范大学,2014[13] 张文慧. 光机械腔系统的动力学行为[D]. 华中师范大学,2014[14]詹孝贵. 腔光机械系统中电磁诱导透明及其相关现象的理论研究[D]. 华中科技大学,20134.毕业论文(设计)应完成的主要内容在阅读大量文献的基础上,完成开题报告,并通过开题答辩。

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a r X i v :c o n d -m a t /0401520v 1 [c o n d -m a t .s t r -e l ] 26 J a n 2004Strong-coupling theory of magnetic-exciton-mediated superconductivity in UPd 2Al 3P.McHaleMax-Planck-Institut f¨u r Physik komplexer Systeme,N¨o thnitzer Str.38,01187Dresden,GermanyP.ThalmeierMax-Planck-Institut f¨u r Chemische Physik fester Stoffe,N¨o thnitzer Str.40,01187Dresden,GermanyP.Fulde Max-Planck-Institut f¨u r Physik komplexer Systeme,N¨o thnitzer Str.38,01187Dresden,Germany (Dated:February 2,2008)There is compelling evidence from inelastic-neutron-scattering and tunneling experiments that the heavy-fermion superconductor UPd 2Al 3can be understood as a dual system consisting of magnetic excitons,arising from crystal-field-split U 4+levels,coupled to delocalised f-electrons.We have computed the superconducting transition temperature and the mass renormalisation arising from a dual model with maximal spin anisotropy using a strong-coupling approach.We find an instability to two possible opposite-spin-pairing states with even-or odd-parity gap functions.Each has a line node perpendicular to the c-direction,in agreement with NMR relaxation-rate,specific-heat and thermal-conductivity measurements.In addition,both have total spin component S z =0,compatible with the observation of a pronounced Knight shift and H c 2Pauli limiting.For parameter values appropriate to UPd 2Al 3,we determine the dependence of the superconducting transition temperature T c on a phenomenological coupling constant g and we investigate the associated mass enhancement and its anisotropy.PACS numbers:74.20.Mn,74.20.Rp I.INTRODUCTION Heavy-fermion superconductors are complicated materials which possess a fascinating and rich variety of physical properties and which have stimulated the creation of an equally diverse range of theories in an effort to understand them.These materials are dominated by strong electronic correlations giving rise to magnetic and superconducting instabilities.Accordingly,most theories ignore phononic degrees of freedom.One of the most extensively studied models of heavy-fermion superconductivity is a phenomenological model based on the exchange of spin fluctuations between heavy quasiparticles.The latter originate in periodic resonant scattering of conduction electrons close to the Fermi level as described within the Kondo lattice model of Ce compounds 1,2.Pairing via spin fluctuations can be considered as a one-component model to the extent that the spin fluctuations originate in the system of heavy quasiparticles and any interaction between conduction electrons and more localised electrons,or conduction electrons and phonons,is neglected.In spite of its simplicity this model has proved to be very useful in our attempts to understand heavy-fermion compounds on the border of magnetic long-range order,such as CePd 2Si 23,CeIn 33and CeRhIn 54.Its success probably derives from the fact that the spin-fluctuation-induced effective interaction tends to dominate all other channels of interaction when a material is tuned close to the border of magnetism by doping or,as in the Ce compounds mentioned above,by applying pressure.The spin-fluctuation mechanism in the Kondo lattice may also be appropriate for the Ce-based heavy-fermion superconductors at ambient pressure,CeCu 2Si 2and CeCoIn 54,5.It has become increasingly evident that the Kondo-lattice model is,however,not adequate in the case of heavy-quasiparticle formation in some Uranium heavy-fermion compounds 6,7,where 5f electrons are partly localised and partly itinerant.The former occupy crystalline-electric-field (CEF)split 5f 2states.The latter,more itinerant,5f electrons have a strongly enhanced effective mass due to a coupling to virtual excitations between CEF states.Thisnotion of heavy-quasiparticle formation is especially appropriate for UPd 2Al 3and it is the starting point of our theoretical model for heavy-fermion superconductivity in this compound.Specifically,we consider a novel effective pairing mechanism which is based on the virtual exchange of collective CEF excitations known as ‘magnetic excitons’.They are propagating bosonic modes in contrast to the overdamped modes which give rise to pairing in the itinerant spin-fluctuation model.The interplay of conduction electrons and CEF excitations is a well studied subject.Initially,research was focused in two areas 8:transport anomalies and superconducting pair breaking or enhancement due to conduction-electron scat-tering from dilute CEF-split impurities;and periodic lattices of CEF ions interacting with one another via conduction-electron polarisation.In the latter case attention was focused on collective effects within the CEF system due to the RKKY interactions mediated by itinerant ter,White and Fulde 9showed that the inverse effect,viz.conduction-electron mass enhancement via virtual emission and absorption of magnetic excitons,is also important.They demonstrated that this mechanism explains the enhanced effective electron masses in praseodymium metal.It is then natural to ask whether the exchange of magnetic excitons between quasiparticles can also mediate superconductivity.Until recently,no theoretical work had been carried out to answer this question,mainly for two reasons.Firstly,when the effects on superconductivity of paramagnetic impurities with CEF-split energy levels were studied in detail 10,it was found that for rare-earth ions the pair-breaking transition matrix elements usually dominate the pair-enhancing matrix elements.Secondly,no good example of a superconducting compound with this dual nature,i.e.,magnetic excitons arising from localised f electrons coupled to delocalised f electrons,was known.Recently,however,evidence has been accumulating that the heavy-fermion compound UPd 2Al 3(T N =14.3K,T c =1.8K,see Ref.11)is the first example where such a mechanism is responsible for superconductivity.Since this mechanism is pair breaking in the s-wave channel (as was already known from the impurity models mentioned above),the superconducting gap function must change sign as a function of k (i.e.,the gap must have a node)as is the case with spin-fluctuation-mediated superconductivity.An early indication that UPd 2Al 3is a localised-delocalised f system came from magnetic-susceptibility measure-ments.Grauel et al 12measured the dc magnetic susceptibility in UPd 2Al 3and argued that the anisotropy which they observed arose from a tetravalent configuration of the Uranium ions,i.e.U 4+(5f 2).Since then Knight-shift 13and optical 14measurements have supported the notion that UPd 2Al 3contains both localised and delocalised f electrons.However,the most direct evidence in favour of the dual-system hypothesis comes from inelastic neutron scattering (INS)and tunnelling experiments.A dispersive crystal-field excitation (magnetic exciton)was observed by Mason and Aeppli 15in INS experiments within the AF ter higher-resolution experiments 16–18revealed a resonance feature which appears in the INS spectrum upon entering the superconducting state.This result demonstrates that a strong interaction exists between the localised and delocalised components of the f-electron system.Pioneering tunnelling experiments 19performed on UPd 2Al 3-AlO x -Pb tunnelling junctions allowed experimenters to view,for the first time,the tunnelling density of states (DOS)of a heavy-fermion superconductor.Strong-coupling features appear in the DOS around 1meV close to the superconducting gap energy reinforcing the view that the exchanged bosons are the magnetic excitons.Taken together,INS and tunnelling experiments lead Sato and co-workers 20to the conclusion that superconductivity arises in this material from an effective interaction between itinerant electrons mediated by magnetic ing a model two-component Hamiltonian they were able to explain qualitative features of the INS scattering spectrum and the superconducting tunnelling spectrum.Subsequently,the origin of the magnetic excitons and their global dispersion,as measured in Ref.15,was investigated in more detail ing an xy-type interaction,where only the σ±components of the conduction-electron spin couples to the magnetic excitons,the effective non-retarded pair potential was derived.The gap equations were solved within a weak-coupling approach demonstrating that the highest T c is obtained by an odd-parity state.In this model,however,the structure of the pairing amplitudes in spin space is complicated,making it unsuitable for going beyond the non-retarded approximation.In this paper,therefore,we investigate an alternative model with a simplified interaction between localised and itinerant 5f electrons.This interaction is of the Ising type,i.e.,only the σz component of the conduction-electron spin can scatter magnetic excitons.In this case,the gap equations naturally divide into those for equal-and opposite-spin pairing,in contrast to the usual ‘singlet’and ‘triplet’classification that arises in spin-rotation-symmetric models.In the present work we treat this simplified dual model for UPd 2Al 3in a more sophisticated strong-coupling ap-proach using a mapping to an electron-boson Hamiltonian and solving the ´Eliashberg equations for the frequency-and momentum-dependent self-energy and gap functions.The level scheme which we use here,and which gives rise to the Ising-type interaction,is quite realistic:recent band-structure calculations based on this level scheme account well for experimental de Haas-van Alphen frequencies in UPd 2Al 37.We demonstrate that our model can yield a super-conducting transition temperature and a mass renormalisation which are consistent with experiment for reasonable values of the coupling constant.II.MODELBand structure calculations based on the supposition that two of the three Uranium 5f-electrons are localised reproduce the observed de Haas-van Alphen frequencies in UPd 2Al 3very well 7.These calculations suggest a level scheme for the localised U 5f states which we adopt here.According to the jj-coupling scheme the U 4+(5f 2)ions have total angular momentum J =4.The twofold degeneracy of the ionic ground state is lifted by a crystalline electric field.We consider only the excitation between the non-degenerate ground state |Γ4 =12(|J z =3 +|J z =−3 ).The CEF energy splitting is of the order ∆≃6meV,asobtained from fitting the magnetic-exciton dispersion obtained from INS 15measurements to theoretical results 21.Although such a model can give rise to induced magnetism via mixing of the states |Γ3 and |Γ4 ,we take theview here that the underlying antiferromagnetic(AF)order is not an important consideration in the description ofheavy-fermion superconductivity in UPd2Al3.AF order mainly leads to a folding down of the conduction bands into the AF Brillouin zone.Also,the magnetic-exciton dispersion in the ordered phase is not appreciably different fromthat in the paramagnetic phase,due to the fact that T N≪∆21.Furthermore,in mean-field theory,the AF order parameter will only slightly modify the superconducting T c due to a reconstruction of the conduction-electron statesclose to the AF Bragg planes.Accordingly we consider a three-dimensional lattice of localised5f2CEF states and itinerant f-electrons.In thesubspace{|Γ3 ,|Γ4 }we may write the CEF part of the Hamiltonian asH CEF=∆ i S iz,(1)where S denotes a pseudospin(S=12 and energy−∆/2and the excited CEF state as having S z=121√2λq αq+α†−q e i qr;λ2q=∆ψβ(r′,τ′) (7)D(r−r′,τ−τ′)=− Tφ(r,τ)φ(r′,τ′) .(8) Note thatφ(r)∼S x(r),as can be seen immediately by comparing the terms∼I in Eqs.(3)and(5),and so D is essentially a pseudospin susceptibility.Furthermore,as in the theory of phonon-mediated superconductivity,φ(r)is real,φ(r)=φ†(r),and commutes with itself,[φ(r),φ(r′)]=0,conditions which allow us to use Wick’s Theorem.The ´Eliashberg equations for the conduction-electron self-energyΣ(p,iω)and gap functionΦ(p,iωn)which follow fromnthe Hamiltonian Eq.(5)areTΣ(p,iωn)=N p′ω′n K(p−p′,iωn−iω′n)|G(p′,iω′n)|2Φ(p′,iω′n).(10)N is the total number of lattice sites.The kernel K is given byK (q ,iνn )=−I 2D 0(q ,iνn )= I 2∆ν2n +ω2q .(11)We have decided not to renormalise D 0by the interaction I between magnetic excitons and electrons.This interaction is,however,already included in D 0to the extent that we model the exciton dispersion ωq by the true experimental dispersion.A particularly noteworthy feature of this formulation is that the effective interaction is dominated by its static part and is strongly peaked in q -space at the antiferromagnetic wavevector Q =(0,0,πc )has actually been observed 17,18in UPd 2Al 3.The electron Green’s function is related to the electron self-energy via the Dysonequation G −1(p ,iωn )=iωn −(ǫp −µ)−Σ(p ,iωn ).(12)The prefactor p in Eq.(10)is the expectation value of the Ising spin-spin interaction ˆσz ˆσz in the spin part of the pair wave function |χ =|S,S z (S here should not be confused with the pseudospin introduced earlier):p = χ|ˆσz ˆσz |χ .(13)In the opposite-spin pair (OSP)states,|χ =12(|↑↓ −|↓↑ )12(|↑↓ +|↓↑ ),(14)p reduces top = ↑↓|ˆσz ˆσz |↑↓ =−1.(15)On the other hand,for each of the equal-spin pair (ESP)states,|χ =|↑↑ and |↓↓ ,p is +1.Note that spin rotational symmetry is broken in a maximal (Ising-type)way in Eq.(10).Consequently the usual classification of pairing states into an (even-parity)singlet with S =0and an (odd-parity)triplet with S =1is no longer valid.In our model,the |1,0 pair state no longer has the same energy as that of the |1,±1 pair states.The result is a different classification into an ESP doublet and two OSP singlet states belonging to irreducible representations of the D 6h group (Table I).Finally,the conduction-band filling,defined as the ratio of the number of electrons to the number of lattice sites,isn =1N z p ′z ω′n K (p z −p ′z ,iωn −iω′n )d p ′⊥N zp ′z ω′n K (p z −p ′z ,iωn −iω′n )Φ(p ′z ,iω′n ) d p ′⊥N z k z Ad k ⊥provided we can carry out the integrals along the perpendicular direction analytically.Here,N z is the number of lattice sites in the z-direction and A is the area of the (hexagonal)unit cell in the plane.We model the exciton dispersion byω(q z )=ωex [1+βcos(q z )];0<β≃1,(21)This form of the dispersion along the c-direction describes qualitatively the observed excitation branch 15.Here 2βωex ≃8meV is the overall dispersion width and (1-β)ωex ≃1meV is the exciton gap at the AF wave vector Q =(0,0,πN z p ′z ω′nK (p z −p ′z ,iωn −iω′n )G z (p ′z ,iω′n )(22)λ(T )Φ(p z ,iωn )=p TN z k z ,ωn >0ln (z ′−1)2+(z ′′)2(ωq z /ωex )2+(νn /ωex )2(25)G ′z (p ′z ,iωn )=−1(z ′)2+(z ′′)2(26)G ′′z (p ′z ,iωn )=− tan −1 1−z ′z ′′(27)M z (p ′z ,iωn )=1z ′′ −tan −1 −z ′2 12π 1TABLE I:Spin and orbital structure of the possible gap functions which are solutions of the´Eliashberg equations for the dual model of UPd2Al3used in this paper.p|χ =|S,S z D6h repres.spin pairingΦ(p z)√√2cos(p′z);α≪1(33) whereαdetermines the degree of corrugation of the FS cylinder along c.The momentum convolutions in Eqs.(22)and(23)were evaluated with the aid of a fast-Fourier-transform algorithm on a32×32lattice.The corresponding frequency sums were carried out using the renormalisation group technique of Pao and Bickers22which allows a considerable reduction of the computational effort.Between240and480Matsubara frequencies were kept at each stage of the renormalisation group procedure.The renormalisation procedure was started at a temperature T0=0.01ǫ⊥and the frequency sum cut-offused wasΩc≈15ǫ⊥.The renormalisation procedure restricts us to discrete temperatures so that the point at which the condition in Eq.(29)is met must be determined by interpolation.The discrete temperatures were sufficiently close that a linear interpolation was adequate.III.RESULTS AND DISCUSSIONScattering by isolated impurities with CEF excitations is usually pair breaking in the s-wave channel8because the dipolar exchange interactions which break the singlet state are stronger than spin-conserving quadrupolar interactions between conduction electrons and CEF states.The s-wave state(whereΦ(p z)is nodeless)is also not favourable in our case of a periodic lattice of partly localised5f-electrons which has dispersive CEF excitations.One can most clearly see this in the following way.In the singlet channel p=−1.Because the kernel K(q,iνn)is strongly peaked at q z=πc)Φ(p z−πc )is a positive number.Therefore afinite gapΦ(p z,iπT)must change sign on translation throughQ z=πc )=−Φ(p z),which excludes an s-wave gap function.However a non-s-wave superconducting state with nodes may take advantage of the exciton dispersion and become stable.From numerical solutions of the linearised gap equations for our model wefind that the instability with the highest T c is accidentally doubly degenerate.The corresponding gap functions transform as the even-and odd-parity OSP states,cos(cp z)and sin(cp z).The former is the usual singlet state;the latter is the S z=0part of the triplet which would appear in a theory with full spin rotational symmetry.We alsofind an instability in the ESP channel but at a much lower temperature.The corresponding pairing symmetry isΦ(p z)∼sin(2cp z).We summarise our results in Table I.The symmetries of the orbital pair wavefunctions can be understood in the following way.By comparing our self-energy equations with those obtained from a four-fermion interaction we see that the effective interaction between quasiparticles in our theory isγ2γ4|ˆV|γ1γ3 =I2D0σzγ1γ2σzγ3γ4,(35) or equivalentlyˆV=I2D0ˆσzˆσz.(36) Hence the pairing interaction in some|χ channel isVχ(q,iνn)= χ|ˆσzˆσz|χ I2D0(q,iνn).(37) We note that our equations go beyond previous calculations6,21in that our formulation includes the full momentum and frequency dependence of the effective interaction Vχ(q,iνn).In the OSP channel the static interaction isV(q z)=−I2D0(q z)=I2∆/2c .The corresponding interaction in real space is therefore attractive when the quasiparti-cles are seperated by a lattice spacing in the c-direction.Now cos(cp z)and sin(cp z)are peaked with equal amplitude in real space at z=c.Hence they are equally well suited to take advantage of the attractive part of the interaction and have equal superconducting transition temperatures.The ESP interaction is the negative of the OSP interaction and so itfirst becomes attractive at z=2c in real space.The only odd-parity wavefunction which is peaked in real space at this position is sin(2cp z).Ultimately,the degeneracy of the OSP states is a peculiarity of the particular CEF level scheme we adopt for the localised5f states and of the approximate form of their exciton dispersion which we assume(viz.strongly wavevector dependent only in the z-direction).Both OSP states are,in fact,compatible with present experimental evidence. OSP states,regardless of the value of total spin angular momentum S,give rise to a reduction in the paramagnetic susceptibility on entering the superconducting state.This reduction comes about because oppositely paired spins have no magnetisation.Furthermore,such a reduction in the Pauli susceptibility leads to an upper criticalfield H c2 which,in some cases,can be smaller than that due to the Meissner effect.This effect is called Pauli limiting23.A pronounced Knight-shift reduction at Pd sites below T c(Refs.13,24)and H c2Pauli-limiting25have both been observed in UPd2Al3.Note also that both OSP gap functions have node lines perpendicular to the c-direction.In the even-parity case they are located at k z=±12N(µ)ǫ⊥12(λ1λ2)2λ3,(40)FIG.1:The dependence of the superconducting transition temperature T c on the coupling constant g[Eq.(30)].The band filling n is0.6.FIG.2:The dependence of the mass renormalisation m∗/m b on the coupling constant g[Eq.(30)].The bandfilling n is0.6 as in Fig.1.m∗min and m∗max are the extremal effective masses over all values of q z.m∗min occurs at q z=0;m∗max occurs at q z=πwhere the dimensionless constantsλi are defined byλ1=IN(µ)(41)λ2=∆/ωex(42)1λ3=)c in UPd2Al3.Solutions of the´Eliashberg equations show that the model favours a superconducting instability for the even-or odd-parity OSP states.Each state has line nodes perpendicular to the c-direction and total z-component of spin S z=0,characteristics which are compatible with measurements of UPd2Al3.Wefind that a superconducting transition temperature and mass renormalisation,each in good agreement with their experimental values in UPd2Al3, can be obtained using reasonable values of the parameters in the theory.Taken together,these results strengthen the argument in favour of a magnetic-exciton system in UPd2Al3.The evidence for dual f-systems in other Uranium compounds does not weigh as heavily as it does in the case of UPd2Al3.In UPt3the number of itinerant f-electrons remains controversial.However band-structure calculations based on the assumption that two of the three5f-electrons are localised reproduce the observed de Haas-van Alphen frequencies as well as the anisotropic heavy electron masses in this compound very well7.Recently unconventional superconductivity with split-T c superconductivity has been discovered in the Pr-based skutterudite PrOs4Sb1233,34.Thermodynamic and transport measurements suggest that the observed heavy-fermion state arises from the interaction of electric quadrupole moments of the CEF-split4f2states of Pr3+with the conduc-tion electrons33.The ground state is probably a singlet and thefirst excited state is probably a triplet,approximately 0.5meV higher,with large off-diagonal quadrupolar matrix elements connecting the two states.The largeness of these matrix elements,together with the very small singlet-triplet splitting,strongly suggests an effective mass renormalisa-tion via virtual CEF excitations.Finally,experiments reveal that the superconducting order parameter is anisotropic, making this compound another candidate for CEF-exciton-mediated superconductivity,but this time of quadrupolar nature.UPd2Al3provides a strong motivation for the study of dual f-electron systems such as the one discussed in this work. We have considered a dual model in which all parameters arefixed except the coupling constant.It will be interesting to investigate the dependence of the transition temperature on conduction-bandfilling and on the form of the exciton dispersion,and to look for a mechanism that can discriminate between the even-and odd-parity superconducting OSP states.AcknowledgmentsP.M.would like to thank P.Monthoux for valuable discussions.P.T.would like to thank K.Maki,Y.Matsuda, K.Izawa,T.Watanabe and G.Varelogiannis for helpful discussions.The authors acknowledge discussions with G. Zwicknagl and A.Yaresko.APPENDIXIn this appendix we sketch the derivation of Eq.(5).Our starting point is the set of Holstein-Primakofftransfor-mations(valid for T≪∆),S z=−12(a+a†)(A.2)Inserting these expressions into the second and third sums in Eq.(3)and Fourier transforming,we arrive at the following form,q W1(q)a†q a q−W2(q)2N kq c†kασzαβc k+qβ(a q+a†−q),(A.3)whereW1(q)=∆−W2(q).(A.4) Thefirst sum can be diagonalised35,while at the same time introducing only a factorλq in the second sum.To do this we use the Bogoliubov transformationαkα†−k = u k v k v k u k a k a†−k,(A.5)where u k=cosh(θk)and v k=sinh(θk).Ifθk is chosen such that−W2(k)/W1(k)=tanh(2θk),(A.6) then(ignoring constant additive terms)thefirst sum in Eq.(A.3)takes the form,qωq(α†qαq+1/2)(A.7) where the dispersionωq satisfiesω2q=W21(q)−W22(q).(A.8) Finally,it is easy to show thata q+a†−q=λq(αq+α†−q),(A.9) whereλq=cosh(θq)−sinh(θq).(A.10) Using Eqs.(A.4)and(A.6),together with the identity∆−2W2(q)=ω2qωq.(A.12) The interaction term in Eq.(5)follows immediately.1A.C.Hewson,The Kondo Problem to Heavy Fermions(Cambridge University Press,1993).11 2P.Fulde,J.Keller,and G.Zwicknagl,in Solid State Physics(Academic Press,San Diego,1988),vol.41,p.1.3N.D.Mathur,F.M.Grosche,S.R.Julian,I.R.Walker,D.M.Freye,R.K.W.Haselwimmer,and G.G.Lonzarich,Nature 394,39(1998).4N.J.Curro,J.L.Sarrao,J.D.Thompson,P.G.Pagliuso,ˇS.Kos,A.Abanov,and D.Pines,Phys.Rev.Lett.90,227202 (2003).5C.Petrovic,P.G.Pagliuso,M.F.Hundley,R.Movshovich,J.L.Sarrao,J.D.Thompson,Z.Fisk,and P.Monthoux,J.Phys.Condens.Matter13,L337(2001).6G.Zwicknagl,A.N.Yaresko,and P.Fulde,Phys.Rev.B65,081103(2002).7G.Zwicknagl,A.Yaresko,and P.Fulde,Phys.Rev.B68,052508(2003).8P.Fulde and I.Peschel,Adv.Phys.21,1(1972).9R.M.White and P.Fulde,Phys.Rev.Lett.47,1540(1981).10P.Fulde,L.L.Hirst,and A.Luther,Z.Phys.230,155(1970).11C.Geibel,C.Schank,S.Thies,H.Kitazawa,C.D.Bredl,A.B¨o hm,M.Rau,A.Grauel,R.Caspary,R.Helfrich,et al.,Z.Phys.B84,1(1991).12A.Grauel,A.B¨o hm,H.Fischer,C.Geibel,R.K¨o hler,R.Modler,C.Schank,F.Steglich,and G.Weber,Phys.Rev.B46, 5818(1992).13R.Feyerherm,A.Amato,F.N.Gygax,A.Schenck,C.Geibel,F.Steglich,N.Sato,and T.Komatsubara,Phys.Rev.Lett.73,1849(1994).14M.Dressel,N.Kasper,K.Pethukhov,B.Gorshunov,G.Gr¨u ner,M.Huth,and H.Adrian,Phys.Rev.Lett.88,186404 (2002).15T.E.Mason and G.Aeppli,Matematisk-fysiske Meddelelser45,231(1997).16N.Sato,N.Aso,nder,B.Roessli,T.Komatsubara,and Y.Endoh,J.Phys.Soc.Japan66,1884(1997).17N.Bernhoeft,N.Sato,B.Roessli,N.Aso,A.Hiess,nder,Y.Endoh,and T.Komatsubara,Phys.Rev.Lett.81, 4244(1998).18N.Bernhoeft,Eur.Phys.J.B13,685(2000).19M.Jourdan,M.Huth,and H.Adrian,Nature398,47(1999).20N.K.Sato,N.Aso,K.Miyake,R.Shiina,P.Thalmeier,G.Varelogiannis,C.Geibel,F.Steglich,P.Fulde,and T.Komat-subara,Nature410,340(2001).21P.Thalmeier,Eur.Phys.J.B27,29(2002).22C.-H.Pao and N.E.Bickers,Phys.Rev.B49,1586(1994).23A.M.Clogston,Phys.Rev.Lett.9,266(1962).24H.Tou,K.Ishida,and Y.Kitaoka,cond-mat/0308562(2003).25J.Hessert,M.Huth,M.Jourdan,H.Adrian,C.T.Rieck,and K.Scharnberg,Physica B230-232,373(1997).26H.Tou,Y.Kitaoka,K.Asayama,C.Geibel,C.Schank,and F.Steglich,Phys.Soc.Jpn.64,725(1995).27K.Matsuda,Y.Kohori,and T.Kohara,Phys.Rev.B55,15223(1997).28N.Sato,unpublished.29M.Hiroi,M.Sera,N.Kobayashi,Y.Haga,E.Yamamoto,and Y.Onuki,J.Phys.Soc.Jpn.66,1595(1997).30P.Thalmeier and K.Maki,Europhys.Lett.58,119(2002).31P.F.J.Jensen,Phys.Rev.B27,4085(1983).32Y.Inada,H.Yamagami,Y.Haga,K.Sakurai,Y.Tokiwa,T.Honma,E.Yamamoto,Y.¯Onuki,and T.Yanagisawa,J.Phys.Soc.Japan68,3643(1999).33E.D.Bauer,N.A.Frederick,P.-C.Ho,V.S.Zapf,and M.B.Maple,Phys.Rev.B65,100506(2002).34R.Vollmer,A.Faisst,C.Pfleiderer,H.v.L¨o hneysen,E.D.Bauer,P.C.Ho,and M.B.Maple,Phys.Rev.Lett.90,57001 (2003).35B.Grover,Phys.Rev.140,A1944(1965).。

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